Adopted components of the solar motion and velocity dispersions
Table
Adopted components of the solar motion and
velocity dispersions
type solar motion (km/sec) spread in velocities (km/sec)
US VS WS U V W
cO–cB5 –9.0 +13.4 +3.7 12 11 9
cF–cM –7.9 +11.7 +6.5 13 9 7
gA –13.4 +11.6 +10.3 22 13 9
gF –19.7 +18.5 +9.5 28 15 9
gG –7.2 +11.1 +6.9 26 18 15
gK0 –10.6 +18.6 +6.5 31 21 16
gK3 –9.0 +17.6 +6.4 31 21 17
gM –4.5 +18.3 +6.2 31 23 16
carbon stars –10.7 +31.8 +3.5 48 23 16
subgiants –8.0 +28.0 +8.0 43 27 24
B0 –9.6 +14.5 +6.7 10 9 6
dA0 –7.3 +13.7 +7.2 15 9 9
dA5 –8.5 +7.8 +7.4 20 9 9
dF5 –10.1 +12.3 +6.2 27 17 17
dG0 –14.5 +21.1 +6.4 26 18 20
dG5 –8.1 +22.1 +4.3 32 17 15
dK0 –10.8 +14.9 +7.4 28 16 11
dK5 –9.5 +22.4 +5.8 35 20 16
dM0 –6.1 +14.6 +6.9 32 21 19
dM5 –9.8 +19.3 +8.6 31 23 16
white dwarfs (white dwarf star) –6 +37 +8 50 33 25
planetary nebulae (planetary nebula) –8 +29 +8 45 35 20
classical Cepheids (Cepheid variable) –8.6 +12.0 +7.6 13 9 5
interstellar Ca II –11.4 +14.4 +8.2 6
See as table:
- Marie Camargo
- Marie-Caroline de Bourbon-Sicile Berry, duchesse de
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- Marie-Catherine Le Jumel de Barneville Aulnoy, Countess d'
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- Marie de Flavigny, comtesse d' Agoult
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- Marie de Rabutin-Chantal Sévigné, marquise de
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- Marie d'Orleans-Longueville Nemours, Duchess de
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